Interstellar neutral hydrogen in the heliosphere

Physics

Scientific paper

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Scientific paper

A fluid model is introduced to study the flow of interstellar neutral hydrogen in the heliosphere. We calculate the normalized density N_H/N_H∞, bulk velocity V_H/V_H∞, and temperature T_H/T_H∞ of interstellar hydrogen as functions of r/lambda and z/lambda where lambda is the ionization scale length. The fluid solution is much less time-consuming than the kinetic theory solutions.

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